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RESULTS FROM THE BO LIQUID ARGON SCINTILLATION TEST STAND AT FERMILAB - PowerPoint PPT Presentation

RESULTS FROM THE BO LIQUID ARGON SCINTILLATION TEST STAND AT FERMILAB Ben Jones, MIT New Perspectives Fermilab, June 11 th 2013 Bo VST Setup Bo Vertical Slice Test is a training ground for one slice of the MicroBooNE optical system


  1. RESULTS FROM THE BO LIQUID ARGON SCINTILLATION TEST STAND AT FERMILAB Ben Jones, MIT New Perspectives Fermilab, June 11 th 2013

  2. Bo VST Setup • Bo Vertical Slice Test is a training ground for one slice of the MicroBooNE optical system including: • Cryogenic photomultiplier tubes • Base electronics • Wavelength shifting plate • High voltage system + interlocks • Cables and splitters • Readout electronics • Cryostat feedthrough • Trace impurity monitors • Etc … uB style PMT • But also a fantastic R&D detector for assembly studying liquid argon scintillation light

  3. 4 Experimental Configuration for This Study

  4. Prompt peak window

  5. Light in Liquid Argon • The scintillation light in liquid argon is produced copiously alongside all ionization charge deposits. � • There are two scintillation pathways, with different time constants – a fast component with t=6ns and a slow time constant with t=1500ns. � γ + 1 Σ u excimer Ar p * * Ar Ar Ar 6ns Ar Ar 1590ns - e 3 Σ u excimer + + Ar p Ar Ar * + e - Ar Ar Ar

  6. Special bonus – possible PID information Ar γ Ar Ar * Scintillation process Ar Ar Ar * Ar Ar Competing Excimer Ar Ar * Dissociation Process Ar Ar • Utlized in dark matter searches (MiniCLEAN, DEAP), and we are investigating the applications of this technique to augment TPC based particle ID in MicroBooNE.

  7. Pulse shape discrimination – a vital tool in dark matter detection, also useful to us!

  8. Fit function for alpha + background Individual components (separated using PSD)

  9. The Effects of Nitrogen in Argon • Unlike oxygen and water, nitrogen does not disturb charge drift in LArTPCs, and is difficult to remove from argon. • Part per million (ppm) levels of dissolved nitrogen are expected to be present in any large future LArTPC detector • Nitrogen at the ppm level leads to : • 1) Scintillation Quenching measured in a detailed study by the WArP collaboration in small test cells (R Acciarri et al 2010 JINST 5 P06003) • 2) Absorption of Scintillation Light Absorption effects of N2 in LAr have not (late light lifetime is affected by N2 – previously been measured So can’t use PSD for this study)

  10. Our Paper (coming soon … )

  11. General Idea: • Source set in one of two possible positions. 14.5” &'()*+',-. #/*0+# • Controlled amounts of N2 injected into the liquid • Quenching affects both source positions equally !"# • Absorption hinders the further more than the nearer source. • If fractional losses from each source deviate we see an N2 absorption length effect. • A future analysis will address the effects $%"# of quenching (more extensively studied by other groups) separately.

  12. • PPM amounts of nitrogen are injected into the liquid from a gas canister, charged to a known pressure. • From known volume of canister and known pressure we can calculate how many ppm we injected. • Nitrogen concentration monitored in both liquid and gas phases using LDetek8000 N2 monitor • We also monitor H20 and O2 to ~10ppb precision from the same sample lines. Trace nitrogen monitor Injection Canister Kindly loaned by Jong Hee Yoo – Thanks!

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

  14. Preliminary Light loss due to N2 in 8” source configuration 27ppb N2 3.7ppm N2 7.4ppm N2 15.5 ppm N2

  15. Attenuation Data Preliminary Divergence of these two lines is clear evidence for the nitrogen absorption effect!

  16. Stability of 1PE - SPE scale stable to within 1% for each run - This is similar to the precision of our SPE measurements - Therefore we assume constant and fold in variations as a systematic error on each point

  17. Just to be sure its really the nitrogen … Preliminary No light loss during periods with no nitrogen injection – gives confidence in system stability, constrains outgassing effects, etc.

  18. Getting to the Attenuation Strength Measured Attenuation Strength: Preliminary Measured Absorption Cross Section:

  19. Comparison to N2 gas absorption cross section world data Preliminary

  20. Nice result, but whats it gonna do for me ? Preliminary $$$$ $

  21. Summary + Prospects • Bo VST has been constructed to test elements of MicroBooNE optical system – also an R&D detector for LAr scintillation light. • Detailed studies of alpha source response have been made and area used in various Bo VST studies • We have measured the effects of nitrogen absorption of 128nm argon scintillation light in liquid argon. We find that the effect is on the order 0.015% / (ppm cm) • This means absorption is no problem for MicroBooNE, and could be useful information for the design of cryo systems for large LArTPCs

  22. Backup Slides

  23. Understanding the Geometrical Effect Ray trace to understand expected light yields per percent of absorption at each position 14.5” 8”

  24. Taking ratio, any quenching effect cancels We will measure the nitrogen absorption effect as % light loss per ppm^-1 cm^-1. Ratio = Light loss at 8” First, measure the light loss ratio as a function of N2 concentration. Light loss at 14.5” In our region of interest the relationship should be ~linear. Absorption strength extracted by comparing the gradient of the measured line to the gradient of the line right, which gives proportionality factor for X axis scales. This factor tells us the % light loss Our region of interest per ppm cm of nitrogen.

  25. How do we know we get N2 concentration right? %#" 70 65 !"#$%&'#$()"*+(,-.#&/*-(0122(344+5( %!" Measured Gas Concentration (ppm) 60 55 50 $#" 45 40 35 $!" 30 25 20 Air Liquide Saturation Tables #" 15 10 NIST REFPROP (Tope) 5 !" 0 0 5 10 15 20 25 !" #" $!" $#" %!" %#" 0#126"#$(7%86%$(9*-&#-'"1/*-(344+5( Measured Liquid Concentration (ppm) 1) Amount of N2 in liquid agrees with 2) Measurement from liquid and gas amount injected to within our uncertainty of capillaries in agreement with saturation the injection volume. pressure based equilibrium calculation

  26. Detected light spectrum – clean Single exponent argon, source at 8” power law (cosmic background) + Poisson (alpha source)

  27. Check on functional form of fits: Power law background is great. Alpha fit needs improvement (not exactly poissonian).

  28. Why? “Shadowing” of outer source edges leads to reduced poisson mean light yield from edge area elements This leads to an enhanced low tail of the source spectrum Disc source kindly loaned by Adam Para – Thanks!

  29. So we Measure the Shadowing Function … Now we know how the source is shadowed, we know how to fit all points.

  30. Improved fit from shadowing function Major improvement with new fit function. Note : no extra free parameters, since shadowing function was tuned on an independent dataset.

  31. Aside: Pulse Shape Discrimination in Action Saturation Alpha Cosmic enriched only

  32. !"#$%&'()*%$& !"#$%&$'()%$&*+,& -#%(.&(,/+.& +,$-./&$)-*#%& 0#*()&%12./(%3&$)-*#%& 4&

  33. PMT Characterizations for MicroBooNE • Measured dark rat

  34. 35 128nm Gehman et al 1.18 ± 0.1 Visible photons out / UV photon in for evaporative TPB

  35. 36 Expected Light Yield at Plate

  36. 37 More ray tracing, should be straightforward enough … • Nope Side view 1/8” Obscured by holder Top view 1” ? 6 mm

  37. 38 Try a few options; System has cylindrical symmetry, so distribution in phi does not matter. Baseline More Obscured Less Obscured 0 < r < 1.5mm : Empty 0 < r < 3mm : Uniform 0 < r < 1.5mm : Uniform 1.5 < r < 3mm : Uniform Source source source 1.5 < r < 3mm : Empty ¾ of plate area covered Full plate area covered ¼ of plate area covered

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